Hostname: page-component-5cf477f64f-zrtmk Total loading time: 0 Render date: 2025-04-04T03:00:46.963Z Has data issue: false hasContentIssue false
  • English
  • Français

High-energy Radiation from a Model of Quasars, AGNs, and the Galactic Center with Magnetic Monopoles

Published online by Cambridge University Press:  25 May 2016

Q.-H. Peng
Q.-H. Peng*
Affiliation:
Department of Astronomy, Nanjing University, Nanjing, 210093, China

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The structural parameters of the supermassive object at the Galactic Center and its high-energy radiation are estimated according to observations in near-infrared radiation, under the model of a supermassive object with magnetic monopoles.

Type
Part II: Posters
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 421 - 422
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Callan, C. 1982, Phys. Rev. D, 25, 2141.CrossRefGoogle Scholar
Eckart, A., & Genzel, R. 1997, MNRAS, 284, 576.CrossRefGoogle Scholar
Gordwurm, A., et al. 1994, Nature, 371, 589.CrossRefGoogle Scholar
Harris, M. J., et al. 1998, ApJ, 501, L55.CrossRefGoogle Scholar
Lingenfelter, R. E., & Ramaty, R. 1989, ApJ, 343, 686.CrossRefGoogle Scholar
Peng, Q. 1989, Ap&SS, 154, 271.Google Scholar
Peng, Q., Wang, D., & Li, Z. 1986, Acta Astrophys. Sinica, 6, 249.Google Scholar
Narayan, R., et al. 1998, ApJ, 492, 554.CrossRefGoogle Scholar
Rubakov, V. 1983, Nucl. Phys. B, 218, 240.CrossRefGoogle Scholar
Swanenburg, B. N., et al. 1981, ApJ, 243, L69.CrossRefGoogle Scholar